Variations of solar ultraviolet irradiance observed by the UARS SOLSTICE -1991 to 1999

Authors
Citation
G. Rottman, Variations of solar ultraviolet irradiance observed by the UARS SOLSTICE -1991 to 1999, SPACE SCI R, 94(1-2), 2000, pp. 83-91
Citations number
11
Categorie Soggetti
Space Sciences
Journal title
SPACE SCIENCE REVIEWS
ISSN journal
00386308 → ACNP
Volume
94
Issue
1-2
Year of publication
2000
Pages
83 - 91
Database
ISI
SICI code
0038-6308(200011)94:1-2<83:VOSUIO>2.0.ZU;2-0
Abstract
The Solar Stellar Irradiance Comparison Experiment (SOLSTICE) is one of ten instruments on the Upper Atmosphere Research Satellite (UARS) - one of two instruments measuring the solar ultraviolet irradiance. The instrument is a three channel spectrometer covering the spectral range 120 to 420 nm with a spectral resolution of approximately 0.2 nm. It has been successfully op erating since October 1991, and has now provided more than eight years of d ata, extending from near the peak of solar cycle 22, through solar minimum and into the new cycle. The data provide time series that display solar var iations over time scales from a few days up to the 11-year solar cycle. Qua ntitative estimates of amplitudes of both rotational modulation and the sol ar cycle variation in the 1991-1999 epoch are given for the UV spectrum bet ween 119 and 300 nm.